Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars: III. Detection of lithium in the metal-poor bulge dwarf MOA-2010-BLG-285S
Bensby, T; Asplund, Martin; Johnson, Jennifer A; Feltzing, Sofia; Melendez, Jorge; Dong, S; Gould, A; Han, C; Aden, Daniel; Lucatello, Sara; Gal-Yam, Avishay
Context. To study the evolution of Li in the Galaxy it is necessary to observe dwarf or subgiant stars. These are the only long-lived stars whose present-day atmospheric chemical composition reflects their natal Li abundances according to standard models
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